Eccentricity evolution in mean motion resonance and non-radial solar wind

Details Eccentricity evolution in mean motion resonance and non-radial solar wind Eccentricity evolution in mean motion resonance and non-radial solar wind

Jul 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009a%26a...501..367p&link_type=abstract

Astronomy and Astrophysics, Volume 501, Issue 1, 2009, pp.367-374

Astronomy and Astrophysics

Astrophysics

1

Sun: Solar Wind, Interplanetary Medium, Celestial Mechanics, Stars: Planetary Systems

Scientific paper

Eccentricity evolution of a dust particle in a mean motion orbital resonance with a planet in circular orbit is investigated. The action of solar electromagnetic and corpuscular radiation, including non-radial components of the solar wind velocity, is taken into account. Various types of eccentricity evolution depend on the angle between the radial direction and the direction of the solar wind velocity. The evolution changes at the analytically derived angles. Its application to exosolar systems is included.

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